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What (who) is loitering$45357$ - definition
![WSO]]](https://commons.wikimedia.org/wiki/Special:FilePath/Delilah missile side.jpg?width=200 "WSO]]")
![[[IAI Harop]], a loitering munition optimized for the [[Suppression of Enemy Air Defenses]] (SEAD) role](https://commons.wikimedia.org/wiki/Special:FilePath/IAI Harop PAS 2013 01.jpg?width=200 "[[IAI Harop]], a loitering munition optimized for the [[Suppression of Enemy Air Defenses]] (SEAD) role")
![[[NCSIST Chien Hsiang]], an example of an expendable loitering munition](https://commons.wikimedia.org/wiki/Special:FilePath/Launcher of Chien hsiang loitering munition.jpg?width=200 "[[NCSIST Chien Hsiang]], an example of an expendable loitering munition")
![[[General Atomics MQ-1 Predator]] [[UCAV]]](https://commons.wikimedia.org/wiki/Special:FilePath/MQ-1 Predator unmanned aircraft.jpg?width=200 "[[General Atomics MQ-1 Predator]] [[UCAV]]")
![XM501]] US prototype capable of launching LAM (loitering attack munition)](https://commons.wikimedia.org/wiki/Special:FilePath/NLOS-LS missile test launch from truck.jpg?width=200 "XM501]] US prototype capable of launching LAM (loitering attack munition)")
![Northrop]] [[AGM-136 Tacit Rainbow]] on display at the National Museum of the U.S. Air Force in Dayton, Ohio](https://commons.wikimedia.org/wiki/Special:FilePath/Northrop AGM-136A Tacit Rainbow.jpg?width=200 "Northrop]] [[AGM-136 Tacit Rainbow]] on display at the National Museum of the U.S. Air Force in Dayton, Ohio")
![[[IAI Harpy]] first-generation loitering munition for SEAD role](https://commons.wikimedia.org/wiki/Special:FilePath/Paris Air Show 2007-06-24 n25.jpg?width=200 "[[IAI Harpy]] first-generation loitering munition for SEAD role")
![Block IV [[Tomahawk cruise missile]]. Its small wing area is optimized for high-speed cruise.](https://commons.wikimedia.org/wiki/Special:FilePath/Tomahawk Block IV cruise missile.jpg?width=200 "Block IV [[Tomahawk cruise missile]]. Its small wing area is optimized for high-speed cruise.")
![Gilbert Wheatley, arrested in England on 7 July 1904, for loitering with intent to commit a [[felony]]](https://commons.wikimedia.org/wiki/Special:FilePath/Gilbert Wheatley, arrested for loitering with intent to commit a felony (23627265035).jpg?width=200 "Gilbert Wheatley, arrested in England on 7 July 1904, for loitering with intent to commit a [[felony]]")
Wikipedia
44 Boötis or i Boötis is a triple star system in the constellation Boötes. It is approximately 41.6 light years from Earth.
44 Boötis can be resolved into two stars, of 5th and 6th magnitudes respectively. They were separated by 1.5″ when the pair were confirmed in 1819, but were only 0.2″ by 2020 as the two orbit every 210 years.
The primary component, 44 Boötis A, is a yellow-white G-type main sequence dwarf with a mean apparent magnitude of +4.83. The companion component, 44 Boötis B, is a W Ursae Majoris variable spectroscopic binary. The variability of this star system was discovered by English astronomer William Herschel. The brightness of the eclipsing binary varies from magnitude +5.8 to +6.40 with a period of 6.43 hours. The two eclipsing components of the are close enough to allow their stellar envelopes to overlap, or at least nearly so.
The 44 Boötis system is 42 light-years (13 parsecs) from Earth. It also may show signs of an infrared excess, implying the existence of a dust disk that absorbs visible light and re-emits it as infrared light. The dust would have a blackbody temperature of about 23 K, situated up to 182 au from the parent star.
